Bahram MOBASHER
(University of California, Riverside)
In this talk we will present the sample of LAEs and LBGs selected in the COSMOS field. Spectroscopic observations of these galaxies are used to confirm their expected redshifts with high success rate. Through SED fitting, we measure the stellar mass, SFR and extinction in these galaxies. A comparison will be carried out between the observed properties of LAEs and LBGs at the same redshift.